Dark matter produced by the freeze-out of inverse decays has a full phase structure, with couplings as small as m_chi over the Planck mass, that is robust to kinetic decoupling and testable through dark photon searches.
Dark Matter from Early Decays
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abstract
Two leading dark matter candidates from supersymmetry and other theories of physics beyond the standard model are WIMPs and weak scale gravitinos. If the lightest stable particle is a gravitino, then a WIMP will decay into it with a natural lifetime of order a month ~ M_{pl}^2/M_{weak}^3. We show that if the bulk of dark matter today came from decays of neutral particles with lifetimes of order a year or smaller, then it could lead to a reduction in the amount of small scale substructure, less concentrated halos and constant density cores in the smallest mass halos. Such beneficial effects may therefore be realized naturally, as discussed by Cembranos, Feng, Rajaraman, and Takayama, in the case of supersymmetry.
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Phases of Dark Matter from Inverse Decays
Dark matter produced by the freeze-out of inverse decays has a full phase structure, with couplings as small as m_chi over the Planck mass, that is robust to kinetic decoupling and testable through dark photon searches.